The discussion explores the relationship between the density of a spinning sphere and the degree of shrinkage of its minor axis. It is noted that the elasticity of the sphere significantly influences this relationship, with faster spinning leading to decreased density and proportional shrinkage of the minor axis. The conversation clarifies that gravity's role is minimal since the sphere is gravity-bound, resulting in an ellipsoidal shape. A denser object exhibits less flattening at a given rotation rate due to stronger gravitational forces. The participants express uncertainty about the exact extent of these effects, particularly in the context of neutron stars.